MAVEN Observes Mars Moon Phobos in the Mid- and Far-Ultraviolet
NASA scientists are closer to solving the mystery of how Mars’ moon Phobos formed. In late November and early December 2015, NASA's Mars Atmosphere and Volatile Evolution (MAVEN) mission made a series of close approaches to the Martian moon Phobos, collecting data from within 300 miles (500 kilometers) of the moon.
The orbit of MAVEN sometimes crosses the orbit of Phobos. This image shows the configuration of the two orbits in early December 2015, when MAVEN's Phobos observations were made.
Credits: CU/LASP and NASA
Among the data returned were spectral images of Phobos in the ultraviolet. The images will allow MAVEN scientists to better assess the composition of this enigmatic object, whose origin is unknown.
Comparing MAVEN's images and spectra of the surface of Phobos to
similar data from asteroids and meteorites will help planetary
scientists understand the moon's origin – whether it is a captured
asteroid or was formed in orbit around Mars. The MAVEN data, when fully
analyzed, will also help scientists look for organic molecules on the
surface. Evidence for such molecules has been reported by previous
measurements from the ultraviolet spectrograph on the Mars Express
spacecraft.
The observations were made by the Imaging Ultraviolet Spectrograph instrument aboard MAVEN.
MAVEN's principal investigator is based at the University of Colorado's Laboratory for Atmospheric and Space Physics, and NASA's Goddard Space Flight Center in Greenbelt, Maryland, manages the MAVEN project. Partner institutions include Lockheed Martin, the University of California at Berkeley, and NASA's Jet Propulsion Laboratory.
For more information on MAVEN, visit:
NASA scientists are closer to solving the mystery of how Mars’ moon Phobos formed. In late November and early December 2015, NASA's Mars Atmosphere and Volatile Evolution (MAVEN) mission made a series of close approaches to the Martian moon Phobos, collecting data from within 300 miles (500 kilometers) of the moon.
Phobos as observed by MAVEN's Imaging Ultraviolet
Spectrograph. Orange shows mid-ultraviolet (MUV) sunlight reflected from
the surface of Phobos, exposing the moon's irregular shape and many
craters. Blue shows far ultraviolet light detected at 121.6 nm, which is
scattered off of hydrogen gas in the extended upper atmosphere of Mars.
Phobos, observed here at a range of 300km, blocks this light, eclipsing
the ultraviolet sky.
Credits: CU/LASP and NASA
The observations were made by the Imaging Ultraviolet Spectrograph instrument aboard MAVEN.
MAVEN's principal investigator is based at the University of Colorado's Laboratory for Atmospheric and Space Physics, and NASA's Goddard Space Flight Center in Greenbelt, Maryland, manages the MAVEN project. Partner institutions include Lockheed Martin, the University of California at Berkeley, and NASA's Jet Propulsion Laboratory.
For more information on MAVEN, visit:
